Showing 41–60 of 79 results
/ Date/ Name
Jan 6, 2024Formation of the Methyl Cation by Photochemistry in a Protoplanetary DiskDec 14, 2023Quantum-centric Supercomputing for Materials Science: A Perspective on Challenges and Future DirectionsOct 11, 2023Chasing Gravitational Waves with the Cherenkov Telescope ArraySep 12, 2023Vortex Fiber Nulling for Exoplanet Observations: Implementation and First LightMay 17, 2023Jet Diffusion versus JetGPT -- Modern Networks for the LHCApr 19, 2023A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z=6.61 QuasarMar 3, 2023IXPE observations of the quintessential wind-accreting X-ray pulsar Vela X-1Mar 2, 2023Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPEDec 7, 2022The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementationAug 2, 2022The CUBES Science CaseJul 14, 2021FOSSIL: I. The Spin Rate Limit of Jupiter TrojansMar 12, 2021Multiwavelength Observations of the RV Tauri Variable System U Monocerotis: Long-Term Variability Phenomena That Can Be Explained by Binary Interactions with a Circumbinary DiskMar 4, 2021Pandemic Drugs at Pandemic Speed: Infrastructure for Accelerating COVID-19 Drug Discovery with Hybrid Machine Learning- and Physics-based Simulations on High Performance ComputersFeb 22, 2021AT 2019qyl in NGC 300: Internal Collisions in the Early Outflow from a Very Fast Nova in a Symbiotic BinaryDec 31, 2020The APOGEE Library of Infrared SSP Templates (A-LIST): High-Resolution Simple Stellar Population Spectral Models in the H-BandOct 29, 2020The FragmentatiOn Of Target Experiment (FOOT) and its DAQ systemDec 27, 2019Quantum Theory of Multisubband Plasmon-Phonon CouplingNov 21, 2019Flat low-loss silicon gradient index lens for millimeter and submillimeter wavelengthsAug 13, 2019The Nearby Evolved Stars Survey: I. JCMT/SCUBA-2 Sub-millimetre detection of the detached shell of U AntliaeAug 13, 2019The Sub-mm Variability of IRC+10216 and $o$ Ceti